Surface roughness
at sub-meter scales remaines unresolved even at the highest available
0.3m/pixel resolution of HiRISE , and is yet a fundamental surface
property of the Martian surface and a pivotal consideration in the
planning stages of lander missions to Mars. This website offers
support for researchers interested in using the 'two-look' roughness
approach described in Mushkin & Gillespie (2005, 2006)
to
map
fine scale surface roughness on Mars.